Kerr-Newman parameters M, a, and Q modulate neutrino survival probabilities, entanglement, and coherence differently from the Schwarzschild case, with spin lengthening and charge shortening oscillation periods in outward radial propagation.
Neutrino oscillations refitted
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abstract
Here we update our previous global fit of neutrino oscillations by including the recent results which have appeared since the Neutrino-2012 conference. These include the measurements of reactor anti-neutrino disappearance reported by Daya Bay and RENO, together with latest T2K and MINOS data including both disappearance and appearance channels. We also include the revised results from the third solar phase of Super-Kamiokande, SK-III, as well as new solar results from the fourth phase of Super-Kamiokande, SK-IV. We find that the preferred global determination of the atmospheric angle $\theta_{23}$ is consistent with maximal mixing. We also determine the impact of the new data upon all the other neutrino oscillation parameters with emphasis on the increasing sensitivity to the CP phase, thanks to the interplay between accelerator and reactor data. In the appendix we present the updated results obtained after the inclusion of new reactor data presented at the Neutrino 2014 conference. We discuss their impact on the global neutrino analysis.
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Quantum Correlations of Neutrinos in the Kerr-Newman Space-time
Kerr-Newman parameters M, a, and Q modulate neutrino survival probabilities, entanglement, and coherence differently from the Schwarzschild case, with spin lengthening and charge shortening oscillation periods in outward radial propagation.
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Updated global fit of neutrino oscillation data gives precise measurements of mixing parameters with a 2.5 sigma preference for normal mass ordering.
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